Search Results - "Pavlenko, Ya"
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Characterization of a Sample of Southern M Dwarfs Using Harps and X-shooter Spectra
Published in The Astrophysical journal (20-06-2019)“…We present the homogeneous analysis of a sample of Southern early-type M dwarfs in the solar neighborhood (d < 60 pc). We used the MCAL technique to derive the…”
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STARSPOT DISTRIBUTIONS ON FULLY CONVECTIVE M DWARFS: IMPLICATIONS FOR RADIAL VELOCITY PLANET SEARCHES
Published in The Astrophysical journal (10-10-2015)“…ABSTRACT Since M4.5-M9 dwarfs exhibit equatorial rotation velocities of the order of 10 km s−1 on average, radial velocity surveys targeting this stellar…”
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The recurrent nova V3890 Sgr: a near-infrared and optical study of the red giant component and its environment
Published in Monthly notices of the Royal Astronomical Society (01-12-2022)“…ABSTRACT We present an analysis of the red giant component of the recurrent nova V3890 Sgr, using data obtained before and after its 2019 eruption. Its…”
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Primeval very low-mass stars and brown dwarfs – VIII. The first age benchmark L subdwarf, a wide companion to a halo white dwarf
Published in Monthly notices of the Royal Astronomical Society (01-09-2024)“…ABSTRACT We report the discovery of five white dwarf + ultracool dwarf systems identified as common proper motion wide binaries in the Gaia Catalogue of Nearby…”
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Rise and fall of silicate dust in RS Ophiuchi following the 2006 eruption
Published in Monthly notices of the Royal Astronomical Society (18-10-2022)“…ABSTRACT We present an analysis of archival Spitzer InfraRed Spectrograph (IRS) observations of the recurrent nova RS Ophiuchi obtained on several occasions,…”
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Primeval very low-mass stars and brown dwarfs – II. The most metal-poor substellar object
Published in Monthly notices of the Royal Astronomical Society (11-06-2017)“…Abstract SDSS J010448.46+153501.8 has previously been classified as an sdM9.5 subdwarf. However, its very blue J − K colour (–0.15 ± 0.17) suggests a much…”
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SiO Bands in the Infrared Spectra of Late-Type Stars
Published in Kinematics and physics of celestial bodies (01-07-2019)“…—The importance of taking the SiO absorption in the infrared spectrum into account for spectral analysis of late-type stars is demonstrated. The lists of…”
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Effective temperatures, rotational velocities, microturbulent velocities and abundances in the atmospheres of the Sun, HD 1835 and HD 10700
Published in Monthly notices of the Royal Astronomical Society (01-05-2012)“…We describe the procedure to determine effective temperatures, rotational velocities, microturbulent velocities and chemical abundances in the atmospheres of…”
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Gas phase SiO in the circumstellar environment of the recurrent nova T Coronae Borealis
Published in Monthly notices of the Royal Astronomical Society (01-07-2019)Get full text
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Improved HCN/HNC linelist, model atmospheres and synthetic spectra for WZ Cas
Published in Monthly notices of the Royal Astronomical Society (01-03-2006)“…We build an accurate data base of 5200 HCN and HNC rotation-vibration energy levels, determined from existing laboratory data. 20 000 energy levels in the…”
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The metal-rich abundance pattern – spectroscopic properties and abundances for 107 main-sequence stars
Published in Monthly notices of the Royal Astronomical Society (01-07-2017)“…Abstract We report results from the high-resolution spectral analysis of the 107 metal-rich (mostly [Fe/H] ≥ 7.67 dex) target stars from the…”
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Determination of abundances in the atmospheres of F-, G-, and K-dwarfs
Published in Kinematics and physics of celestial bodies (01-03-2017)“…The algorithm of the determination of abundances in atmospheres of stars of spectral classes F, G, and K using fits to the observed spectral lines or selected…”
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Old Stars in Young Clusters: Lithium-depleted Low-Mass Stars of the Orion Nebula Cluster
Published in The Astrophysical journal (10-04-2007)“…We measured lithium in a sample of low-mass stars (60.1-0.3 M sub((m=o.))) of the Orion Nebula cluster. We find evidence for significant Li depletion in four…”
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Erratum: Gas phase SiO in the circumstellar environment of the recurrent nova T Coronae Borealis
Published in Monthly notices of the Royal Astronomical Society (01-05-2022)Get full text
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A spectroscopic and proper motion search of Sloan Digital Sky Survey: red subdwarfs in binary systems
Published in Monthly notices of the Royal Astronomical Society (11-09-2013)“…Red subdwarfs in binary systems are crucial for both model calibration and spectral classification. We search for red subdwarfs in binary systems from a sample…”
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Molecular bands in the spectra of M stars
Published in Astronomy reports (01-11-2014)“…The profiles of the main molecular bands in the spectral-energy distributions (SEDs) of M stars have been calculated. The calculations of the individual band…”
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Analysis of Actinium Abundances in the Atmosphere of Cepheid HIP13962
Published in Kinematics and physics of celestial bodies (01-04-2022)“…Actinium is a radioactive element that has an isotope 227 Ac with the longest half-life of 21.772(3) years. It is the third element in the actinoid group, in…”
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Modelling the spectral energy distribution of the red giant in RS Ophiuchi: evidence for irradiation
Published in Monthly notices of the Royal Astronomical Society (11-02-2016)“…We present an analysis of optical and infrared spectra of the recurrent nova RS Oph obtained during between 2006 and 2009. The best fit to the optical spectrum…”
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Collision-induced absorption of radiation in the atmospheres of late-type stars
Published in Astronomy reports (01-05-2016)“…Problems associated with taking into account absorption induced by collisions between hydrogen and helium atoms, helium atoms and hydrogen molecules, and…”
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